PMO OpenIR
multiwavelengthstudyoflowluminosity67ghzmethanolmasers
Wu Yuanwei; Xu Ye; Yang Ji
2011
Source Publicationresearchinastronomyandastrophysics
ISSN1674-4527
Volume11Issue:2Pages:137
AbstractWe present results of ~(13)CO(1-0),C~(18)O(1-0), and HCO~+(1-0)map observations and N_2H~+(1-0)single point observations directed towards a sample of nine low-luminosity 6.7-GHz masers. N_2H~+line emission has been detected from six out of nine sources,C~(18)O line emission has been detected from eight out of nine sources, and HCO~+ and ~(13)CO emission has been detected in all sources. In particular, a"blue profile"of the HCO~+ spectrum,a signature of inflow,is found towards one source. From integrated intensity emission maps,we identified 17 cores in the sample. Among them, nine cores are closely associated with low-luminosity methanol masers. For these cores,we derive the column densities, core sizes, masses and molecular abundances. Comparison of our results with similar molecular line surveys towards the southern sky methanol masers indicates that linewidths of our sample, including only the low-luminosity masers, are smaller than the sample that includes both lowand high-luminosity masers. For the maser associated cores, their gas masses have the same order of magnitude as their virial masses, indicating that these cores are gravitationally bound systems. In addition,we have found from our observations that the low-luminosity methanol masers tend to coexist with H_2O masers and outflows rather than with OH masers
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/30803
Collection中国科学院紫金山天文台
Affiliation中国科学院紫金山天文台
First Author Affilication中国科学院紫金山天文台
Recommended Citation
GB/T 7714
Wu Yuanwei,Xu Ye,Yang Ji. multiwavelengthstudyoflowluminosity67ghzmethanolmasers[J]. researchinastronomyandastrophysics,2011,11(2):137.
APA Wu Yuanwei,Xu Ye,&Yang Ji.(2011).multiwavelengthstudyoflowluminosity67ghzmethanolmasers.researchinastronomyandastrophysics,11(2),137.
MLA Wu Yuanwei,et al."multiwavelengthstudyoflowluminosity67ghzmethanolmasers".researchinastronomyandastrophysics 11.2(2011):137.
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